An alpha particle (mass \(=4.00 \mathrm{u}\) ) has a head-on, elastic collision with a nucleus (mass \(=166 \mathrm{u}\) ) that is initially at rest. What percentage of the kinetic energy of the alpha particle is transferred to the nucleus in the collision?

Short Answer

Expert verified
Answer: To calculate the percentage of kinetic energy transferred, we need the initial or final velocities of the alpha particle, which were not provided in this exercise. If such values were provided or could be calculated from given information, the remaining calculations could be completed using the conservation of momentum and conservation of energy equations to find the percentage of kinetic energy transferred.

Step by step solution

01

Conservation of Momentum

According to the law of conservation of momentum, the total momentum of the system before the collision equals the total momentum of the system after the collision. Let's denote the masses of alpha particle and nucleus as m1 and m2 respectively, and their initial and final velocities as u1, u2, v1, and v2 respectively. Since the nucleus is initially at rest, u2 = 0. Initially, Momentum of alpha particle = m1u1 Initially, Momentum of nucleus = m2u2 (which is 0) Finally, Momentum of alpha particle = m1v1 Finally, Momentum of nucleus = m2v2 Conservation of momentum equation can be written as: m1u1 + m2u2 = m1v1 + m2v2 Plugging in the known values, we get: m1u1 = m1v1 + m2v2
02

Conservation of Energy

For an elastic collision, the total mechanical energy is conserved. Hence, the initial kinetic energy (KE_initial) equals the final kinetic energy (KE_final). KE_initial = KE_final Initial kinetic energy of alpha particle = \(\frac{1}{2}m1u1^2\) Initial kinetic energy of nucleus = 0 (since it's initially at rest) Final kinetic energy of alpha particle = \(\frac{1}{2}m1v1^2\) Final kinetic energy of nucleus = \(\frac{1}{2}m2v2^2\) Now, equating the initial and final kinetic energies, we get: \(\frac{1}{2}m1u1^2 = \frac{1}{2}m1v1^2 + \frac{1}{2}m2v2^2\)
03

Solve for v2

To find the percentage of kinetic energy transferred, we need to find the final velocity of the nucleus (v2) after the collision. Using the conservation of momentum equation from Step 1, we can solve for v2: v2 = \(\frac{m1(u1-v1)}{m2}\)
04

Substitute values and find the percentage of transferred kinetic energy

The mass of alpha particle m1 = 4.00 u and mass of nucleus m2 = 166 u. Calculate the final kinetic energy of the nucleus by substituting the values: KE_final_nucleus = \(\frac{1}{2}m2v2^2\) Percentage of kinetic energy transferred = \(\frac{KE_{final\_nucleus}}{KE_{initial}}\) × 100 Plug in the values and compute the final answer. Note that we have not been provided the initial or final velocities of the alpha particle. If such values were provided or could be calculated from given information, the remaining calculations could be completed to find the percentage of kinetic energy transferred.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

NASA has taken an increased interest in near Earth asteroids. These objects, popularized in recent blockbuster movies, can pass very close to Earth on a cosmic scale, sometimes as close as 1 million miles. Most are small-less than \(500 \mathrm{~m}\) across \(-\) and while an impact with one of the smaller ones could be dangerous, experts believe that it may not be catastrophic to the human race. One possible defense system against near Earth asteroids involves hitting an incoming asteroid with a rocket to divert its course. Assume a relatively small asteroid with a mass of \(2.10 \cdot 10^{10} \mathrm{~kg}\) is traveling toward the Earth at a modest speed of \(12.0 \mathrm{~km} / \mathrm{s}\). a) How fast would a large rocket with a mass of \(8.00 \cdot 10^{4} \mathrm{~kg}\) have to be moving when it hit the asteroid head on in order to stop the asteroid? b) An alternative approach would be to divert the asteroid from its path by a small amount to cause it to miss Earth. How fast would the rocket of part (a) have to be traveling at impact to divert the asteroid's path by \(1.00^{\circ}\) ? In this case, assume that the rocket hits the asteroid while traveling along a line perpendicular to the asteroid's path.

Cosmic rays from space that strike Earth contain some charged particles with energies billions of times higher than any that can be produced in the biggest accelerator. One model that was proposed to account for these particles is shown schematically in the figure. Two very strong sources of magnetic fields move toward each other and repeatedly reflect the charged particles trapped between them. (These magnetic field sources can be approximated as infinitely heavy walls from which charged particles get reflected elastically.) The high- energy particles that strike the Earth would have been reflected a large number of times to attain the observed energies. An analogous case with only a few reflections demonstrates this effect. Suppose a particle has an initial velocity of \(-2.21 \mathrm{~km} / \mathrm{s}\) (moving in the negative \(x\) -direction, to the left), the left wall moves with a velocity of \(1.01 \mathrm{~km} / \mathrm{s}\) to the right, and the right wall moves with a velocity of \(2.51 \mathrm{~km} / \mathrm{s}\) to the left. What is the velocity of the particle after six collisions with the left wall and five collisions with the right wall?

Astronauts are playing catch on the International Space Station. One 55.0 -kg astronaut, initially at rest, throws a baseball of mass \(0.145 \mathrm{~kg}\) at a speed of \(31.3 \mathrm{~m} / \mathrm{s}\). At what speed does the astronaut recoil?

An 83.0 -kg running back leaps straight ahead toward the end zone with a speed of \(6.50 \mathrm{~m} / \mathrm{s}\). A 115 -kg linebacker, keeping his feet on the ground, catches the running back and applies a force of \(900 . \mathrm{N}\) in the opposite direction for 0.750 s before the running back's feet touch the ground. a) What is the impulse that the linebacker imparts to the running back? b) What change in the running back's momentum does the impulse produce? c) What is the running back's momentum when his feet touch the ground? d) If the linebacker keeps applying the same force after the running back's feet have touched the ground, is this still the only force acting to change the running back's momentum?

A soccer ball rolls out of a gym through the center of a doorway into the next room. The adjacent room is \(6.00 \mathrm{~m}\) by \(6.00 \mathrm{~m}\) with the \(2.00-\mathrm{m}\) wide doorway located at the center of the wall. The ball hits the center of a side wall at \(45.0^{\circ} .\) If the coefficient of restitution for the soccer ball is \(0.700,\) does the ball bounce back out of the room? (Note that the ball rolls without slipping, so no energy is lost to the floor.)

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free